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description Publicationkeyboard_double_arrow_right Article , Preprint , Other literature type , Journal 2018Embargo end date: 01 Jan 2018 United Kingdom, France, France, France, France, Poland, France, France, France, Germany, Germany, France, Germany, Italy, Netherlands, France, France, Germany, France, France, South Africa, France, France, South AfricaPublisher:EDP Sciences Publicly fundedFunded by:EC | PRECISIONGAMMA, DFGEC| PRECISIONGAMMA ,DFGCollaboration, H. E. S. S.; Abdalla, H.; Abramowski, A.; Aharonian, F.; Benkhali, F. Ait; Ang��ner, E. O.; Arakawa, M.; Arrieta, M.; Aubert, P.; Backes, M.; Balzer, A.; Barnard, M.; Becherini, Y.; Tjus, J. Becker; Berge, D.; Bernhard, S.; Bernl��hr, K.; Blackwell, R.; B��ttcher, M.; Boisson, C.; Bolmont, J.; Bonnefoy, S.; Bordas, P.; Bregeon, J.; Brun, F.; Brun, P.; Bryan, M.; B��chele, M.; Bulik, T.; Capasso, M.; Caroff, S.; Carosi, A.; Casanova, S.; Cerruti, M.; Chakraborty, N.; Chaves, R. C. G.; Chen, A.; Chevalier, J.; Colafrancesco, S.; Condon, B.; Conrad, J.; Davids, I. D.; Decock, J.; Deil, C.; Devin, J.; deWilt, P.; Dirson, L.; Djannati-Ata��, A.; Domainko, W.; Donath, A.; Drury, L. O'C.; Dutson, K.; Dyks, J.; Edwards, T.; Egberts, K.; Eger, P.; Emery, G.; Ernenwein, J. -P.; Eschbach, S.; Farnier, C.; Fegan, S.; Fernandes, M. V.; Fiasson, A.; Fontaine, G.; F��rster, A.; Funk, S.; F����ling, M.; Gabici, S.; Gallant, Y. A.; Garrigoux, T.; Gat��, F.; Giavitto, G.; Giebels, B.; Glawion, D.; Glicenstein, J. F.; Gottschall, D.; Grondin, M. -H.; Hahn, J.; Haupt, M.; Hawkes, J.; Heinzelmann, G.; Henri, G.; Hermann, G.; Hinton, J. A.; Hofmann, W.; Hoischen, C.; Holch, T. L.; Holler, M.; Horns, D.; Ivascenko, A.; Iwasaki, H.; Jacholkowska, A.; Jamrozy, M.; Jankowsky, D.; Jankowsky, F.; Jingo, M.; Jouvin, L.; Jung-Richardt, I.; Kastendieck, M. A.; Katarzy��ski, K.; Katsuragawa, M.; Katz, U.; Kerszberg, D.; Khangulyan, D.; Kh��lifi, B.; King, J.; Klepser, S.; Klochkov, D.; Klu��niak, W.; Komin, Nu.; Kosack, K.; Krakau, S.; Kraus, M.; Kr��ger, P. P.; Laffon, H.; Lamanna, G.; Lau, J.; Lees, J. -P.; Lefaucheur, J.; Lemi��re, A.; Lemoine-Goumard, M.; Lenain, J. -P.; Leser, E.; Lohse, T.; Lorentz, M.; Liu, R.; L��pez-Coto, R.; Lypova, I.; Malyshev, D.; Marandon, V.; Marcowith, A.; Mariaud, C.; Marx, R.; Maurin, G.; Maxted, N.; Mayer, M.; Meintjes, P. J.; Meyer, M.; Mitchell, A. M. W.; Moderski, R.; Mohamed, M.; Mohrmann, L.; Mor��, K.; Moulin, E.; Murach, T.; Nakashima, S.; de Naurois, M.; Ndiyavala, H.; Niederwanger, F.; Niemiec, J.; Oakes, L.; O'Brien, P.; Odaka, H.; Ohm, S.; Ostrowski, M.; Oya, I.; Padovani, M.; Panter, M.; Parsons, R. D.; Pekeur, N. W.; Pelletier, G.; Perennes, C.; Petrucci, P. -O.; Peyaud, B.; Piel, Q.; Pita, S.; Poireau, V.; Poon, H.; Prokhorov, D.; Prokoph, H.; P��hlhofer, G.; Punch, M.; Quirrenbach, A.; Raab, S.; Rauth, R.; Reimer, A.; Reimer, O.; Renaud, M.; Reyes, R. de los; Rieger, F.; Rinchiuso, L.; Romoli, C.; Rowell, G.; Rudak, B.; Rulten, C. B.; Sahakian, V.; Saito, S.; Sanchez, D. A.; Santangelo, A.; Sasaki, M.; Schandri, M.; Schlickeiser, R.; Sch��ssler, F.; Schulz, A.; Schwanke, U.; Schwemmer, S.; Seglar-Arroyo, M.; Settimo, M.; Seyffert, A. S.; Shafi, N.;Context. Recently, the high-energy (HE, 0.1–100 GeV) γ-ray emission from the object LMC P3 in the Large Magellanic Cloud (LMC) has been discovered to be modulated with a 10.3-day period, making it the first extra-galactic γ-ray binary. Aim. This work aims at the detection of very-high-energy (VHE, >100 GeV) γ-ray emission and the search for modulation of the VHE signal with the orbital period of the binary system. Methods. LMC P3 has been observed with the High Energy Stereoscopic System (H.E.S.S.); the acceptance-corrected exposure time is 100 h. The data set has been folded with the known orbital period of the system in order to test for variability of the emission. Results. VHE γ-ray emission is detected with a statistical significance of 6.4 σ. The data clearly show variability which is phase-locked to the orbital period of the system. Periodicity cannot be deduced from the H.E.S.S. data set alone. The orbit-averaged luminosity in the 1–10 TeV energy range is (1.4 ± 0.2) × 1035 erg s−1. A luminosity of (5 ± 1) × 1035 erg s−1 is reached during 20% of the orbit. HE and VHE γ-ray emissions are anti-correlated. LMC P3 is the most luminous γ-ray binary known so far.
North-West Universit... arrow_drop_down North-West University, South Africa: Boloka (NWU-IR)Article . 2018Full-Text: http://hdl.handle.net/10394/26678Data sources: Bielefeld Academic Search Engine (BASE)Astronomy and AstrophysicsOther literature type . 2018Data sources: Universiteit van Amsterdam Digital Academic RepositoryOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2018Data sources: OA@INAF - Istituto Nazionale di AstrofisicaINRIA a CCSD electronic archive serverArticle . 2018Data sources: INRIA a CCSD electronic archive serverÉcole Polytechnique, Université Paris-Saclay: HALArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Institut National de la Recherche Agronomique: ProdINRAArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2018Data sources: Bielefeld Academic Search Engine (BASE)Universiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2018Data sources: Bielefeld Academic Search Engine (BASE)Astronomy and AstrophysicsArticle . 2018 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyData sources: CrossrefPublikationsserver der Universität PotsdamArticle . 2018Data sources: Publikationsserver der Universität Potsdamhttps://dx.doi.org/10.48550/ar...Article . 2018License: arXiv Non-Exclusive DistributionData sources: DataciteÉcole Polytechnique, Université Paris-Saclay: HALArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Eberhard Karls University Tübingen: Publication SystemArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2018Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1051/0004-6361/201732426&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 13 citations 13 popularity Top 10% influence Average impulse Top 10% 
Powered by BIP!more_vert North-West Universit... arrow_drop_down North-West University, South Africa: Boloka (NWU-IR)Article . 2018Full-Text: http://hdl.handle.net/10394/26678Data sources: Bielefeld Academic Search Engine (BASE)Astronomy and AstrophysicsOther literature type . 2018Data sources: Universiteit van Amsterdam Digital Academic RepositoryOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2018Data sources: OA@INAF - Istituto Nazionale di AstrofisicaINRIA a CCSD electronic archive serverArticle . 2018Data sources: INRIA a CCSD electronic archive serverÉcole Polytechnique, Université Paris-Saclay: HALArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Institut National de la Recherche Agronomique: ProdINRAArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2018Data sources: Bielefeld Academic Search Engine (BASE)Universiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2018Data sources: Bielefeld Academic Search Engine (BASE)Astronomy and AstrophysicsArticle . 2018 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyData sources: CrossrefPublikationsserver der Universität PotsdamArticle . 2018Data sources: Publikationsserver der Universität Potsdamhttps://dx.doi.org/10.48550/ar...Article . 2018License: arXiv Non-Exclusive DistributionData sources: DataciteÉcole Polytechnique, Université Paris-Saclay: HALArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Eberhard Karls University Tübingen: Publication SystemArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2018Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1051/0004-6361/201732426&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Conference object , Article , Preprint , Other literature type , Journal 2020Embargo end date: 01 Jan 2020 France, Spain, Spain, SpainPublisher:Sissa Medialab Funded by:ANR | SUPER, UKRI | Materia Oscura: Instrumen..., SNSF | The search for dark matte... +1 projectsANR| SUPER ,UKRI| Materia Oscura: Instrumentation Development to Observe the Invisible ,SNSF| The search for dark matter using CCD detectors (DAMIC) ,NSF| The Search for Light Dark Matter with DAMICA. Aguilar-Arevalo; D. Amidei; D. Baxter; G. Cancelo; B. A. Cervantes Vergara; A. E. Chavarria; J. C. D’Olivo; J. Estrada; F. Favela-Perez; R. Gaïor; Y. Guardincerri; E. W. Hoppe; T. W. Hossbach; B. Kilminster; I. Lawson; S. J. Lee; A. Letessier-Selvon; A. Matalon; P. Mitra; C. T. Overman; A. Piers; P. Privitera; K. Ramanathan; J. Da Rocha; Y. Sarkis; M. Settimo; R. Smida; R. Thomas; J. Tiffenberg; M. Traina; R. Vilar; A. L. Virto;pmid: 33412014
handle: 10261/229942 , 10902/28225
We present constraints on the existence of weakly interacting massive particles (WIMPs) from an 11 kg-day target exposure of the DAMIC experiment at the SNOLAB underground laboratory. The observed energy spectrum and spatial distribution of ionization events with electron-equivalent energies $>$200 eV$_{\rm ee}$ in the DAMIC CCDs are consistent with backgrounds from natural radioactivity. An excess of ionization events is observed above the analysis threshold of 50 eV$_{\rm ee}$. While the origin of this low-energy excess requires further investigation, our data exclude spin-independent WIMP-nucleon scattering cross sections $��_{��-n}$ as low as $3\times 10^{-41}$ cm$^2$ for WIMPs with masses $m_��$ from 7 to 10 GeV$c^{-2}$ . These results are the strongest constraints from a silicon target on the existence of WIMPs with $m_��$$ 6 pages, 4 figures
https://pos.sissa.it... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAArticle . 2020 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAConference object . 2022License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAMémoires en Sciences de l'Information et de la CommunicationConference object . 2021Physical Review LettersArticle . 2020 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useData sources: Crossrefhttps://dx.doi.org/10.48550/ar...Article . 2020License: arXiv Non-Exclusive DistributionData sources: DataciteUniversité de Nantes: HAL-UNIV-NANTESArticle . 2020Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.22323/1.395.0539&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 63 citations 63 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!visibility 42visibility views 42 download downloads 114 Powered by
more_vert https://pos.sissa.it... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAArticle . 2020 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAConference object . 2022License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAMémoires en Sciences de l'Information et de la CommunicationConference object . 2021Physical Review LettersArticle . 2020 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useData sources: Crossrefhttps://dx.doi.org/10.48550/ar...Article . 2020License: arXiv Non-Exclusive DistributionData sources: DataciteUniversité de Nantes: HAL-UNIV-NANTESArticle . 2020Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.22323/1.395.0539&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eu
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description Publicationkeyboard_double_arrow_right Article , Preprint , Other literature type , Journal 2018Embargo end date: 01 Jan 2018 United Kingdom, France, France, France, France, Poland, France, France, France, Germany, Germany, France, Germany, Italy, Netherlands, France, France, Germany, France, France, South Africa, France, France, South AfricaPublisher:EDP Sciences Publicly fundedFunded by:EC | PRECISIONGAMMA, DFGEC| PRECISIONGAMMA ,DFGCollaboration, H. E. S. S.; Abdalla, H.; Abramowski, A.; Aharonian, F.; Benkhali, F. Ait; Ang��ner, E. O.; Arakawa, M.; Arrieta, M.; Aubert, P.; Backes, M.; Balzer, A.; Barnard, M.; Becherini, Y.; Tjus, J. Becker; Berge, D.; Bernhard, S.; Bernl��hr, K.; Blackwell, R.; B��ttcher, M.; Boisson, C.; Bolmont, J.; Bonnefoy, S.; Bordas, P.; Bregeon, J.; Brun, F.; Brun, P.; Bryan, M.; B��chele, M.; Bulik, T.; Capasso, M.; Caroff, S.; Carosi, A.; Casanova, S.; Cerruti, M.; Chakraborty, N.; Chaves, R. C. G.; Chen, A.; Chevalier, J.; Colafrancesco, S.; Condon, B.; Conrad, J.; Davids, I. D.; Decock, J.; Deil, C.; Devin, J.; deWilt, P.; Dirson, L.; Djannati-Ata��, A.; Domainko, W.; Donath, A.; Drury, L. O'C.; Dutson, K.; Dyks, J.; Edwards, T.; Egberts, K.; Eger, P.; Emery, G.; Ernenwein, J. -P.; Eschbach, S.; Farnier, C.; Fegan, S.; Fernandes, M. V.; Fiasson, A.; Fontaine, G.; F��rster, A.; Funk, S.; F����ling, M.; Gabici, S.; Gallant, Y. A.; Garrigoux, T.; Gat��, F.; Giavitto, G.; Giebels, B.; Glawion, D.; Glicenstein, J. F.; Gottschall, D.; Grondin, M. -H.; Hahn, J.; Haupt, M.; Hawkes, J.; Heinzelmann, G.; Henri, G.; Hermann, G.; Hinton, J. A.; Hofmann, W.; Hoischen, C.; Holch, T. L.; Holler, M.; Horns, D.; Ivascenko, A.; Iwasaki, H.; Jacholkowska, A.; Jamrozy, M.; Jankowsky, D.; Jankowsky, F.; Jingo, M.; Jouvin, L.; Jung-Richardt, I.; Kastendieck, M. A.; Katarzy��ski, K.; Katsuragawa, M.; Katz, U.; Kerszberg, D.; Khangulyan, D.; Kh��lifi, B.; King, J.; Klepser, S.; Klochkov, D.; Klu��niak, W.; Komin, Nu.; Kosack, K.; Krakau, S.; Kraus, M.; Kr��ger, P. P.; Laffon, H.; Lamanna, G.; Lau, J.; Lees, J. -P.; Lefaucheur, J.; Lemi��re, A.; Lemoine-Goumard, M.; Lenain, J. -P.; Leser, E.; Lohse, T.; Lorentz, M.; Liu, R.; L��pez-Coto, R.; Lypova, I.; Malyshev, D.; Marandon, V.; Marcowith, A.; Mariaud, C.; Marx, R.; Maurin, G.; Maxted, N.; Mayer, M.; Meintjes, P. J.; Meyer, M.; Mitchell, A. M. W.; Moderski, R.; Mohamed, M.; Mohrmann, L.; Mor��, K.; Moulin, E.; Murach, T.; Nakashima, S.; de Naurois, M.; Ndiyavala, H.; Niederwanger, F.; Niemiec, J.; Oakes, L.; O'Brien, P.; Odaka, H.; Ohm, S.; Ostrowski, M.; Oya, I.; Padovani, M.; Panter, M.; Parsons, R. D.; Pekeur, N. W.; Pelletier, G.; Perennes, C.; Petrucci, P. -O.; Peyaud, B.; Piel, Q.; Pita, S.; Poireau, V.; Poon, H.; Prokhorov, D.; Prokoph, H.; P��hlhofer, G.; Punch, M.; Quirrenbach, A.; Raab, S.; Rauth, R.; Reimer, A.; Reimer, O.; Renaud, M.; Reyes, R. de los; Rieger, F.; Rinchiuso, L.; Romoli, C.; Rowell, G.; Rudak, B.; Rulten, C. B.; Sahakian, V.; Saito, S.; Sanchez, D. A.; Santangelo, A.; Sasaki, M.; Schandri, M.; Schlickeiser, R.; Sch��ssler, F.; Schulz, A.; Schwanke, U.; Schwemmer, S.; Seglar-Arroyo, M.; Settimo, M.; Seyffert, A. S.; Shafi, N.;Context. Recently, the high-energy (HE, 0.1–100 GeV) γ-ray emission from the object LMC P3 in the Large Magellanic Cloud (LMC) has been discovered to be modulated with a 10.3-day period, making it the first extra-galactic γ-ray binary. Aim. This work aims at the detection of very-high-energy (VHE, >100 GeV) γ-ray emission and the search for modulation of the VHE signal with the orbital period of the binary system. Methods. LMC P3 has been observed with the High Energy Stereoscopic System (H.E.S.S.); the acceptance-corrected exposure time is 100 h. The data set has been folded with the known orbital period of the system in order to test for variability of the emission. Results. VHE γ-ray emission is detected with a statistical significance of 6.4 σ. The data clearly show variability which is phase-locked to the orbital period of the system. Periodicity cannot be deduced from the H.E.S.S. data set alone. The orbit-averaged luminosity in the 1–10 TeV energy range is (1.4 ± 0.2) × 1035 erg s−1. A luminosity of (5 ± 1) × 1035 erg s−1 is reached during 20% of the orbit. HE and VHE γ-ray emissions are anti-correlated. LMC P3 is the most luminous γ-ray binary known so far.
North-West Universit... arrow_drop_down North-West University, South Africa: Boloka (NWU-IR)Article . 2018Full-Text: http://hdl.handle.net/10394/26678Data sources: Bielefeld Academic Search Engine (BASE)Astronomy and AstrophysicsOther literature type . 2018Data sources: Universiteit van Amsterdam Digital Academic RepositoryOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2018Data sources: OA@INAF - Istituto Nazionale di AstrofisicaINRIA a CCSD electronic archive serverArticle . 2018Data sources: INRIA a CCSD electronic archive serverÉcole Polytechnique, Université Paris-Saclay: HALArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Institut National de la Recherche Agronomique: ProdINRAArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2018Data sources: Bielefeld Academic Search Engine (BASE)Universiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2018Data sources: Bielefeld Academic Search Engine (BASE)Astronomy and AstrophysicsArticle . 2018 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyData sources: CrossrefPublikationsserver der Universität PotsdamArticle . 2018Data sources: Publikationsserver der Universität Potsdamhttps://dx.doi.org/10.48550/ar...Article . 2018License: arXiv Non-Exclusive DistributionData sources: DataciteÉcole Polytechnique, Université Paris-Saclay: HALArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Eberhard Karls University Tübingen: Publication SystemArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2018Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1051/0004-6361/201732426&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 13 citations 13 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert North-West Universit... arrow_drop_down North-West University, South Africa: Boloka (NWU-IR)Article . 2018Full-Text: http://hdl.handle.net/10394/26678Data sources: Bielefeld Academic Search Engine (BASE)Astronomy and AstrophysicsOther literature type . 2018Data sources: Universiteit van Amsterdam Digital Academic RepositoryOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2018Data sources: OA@INAF - Istituto Nazionale di AstrofisicaINRIA a CCSD electronic archive serverArticle . 2018Data sources: INRIA a CCSD electronic archive serverÉcole Polytechnique, Université Paris-Saclay: HALArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Institut National de la Recherche Agronomique: ProdINRAArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2018Data sources: Bielefeld Academic Search Engine (BASE)Universiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2018Data sources: Bielefeld Academic Search Engine (BASE)Astronomy and AstrophysicsArticle . 2018 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyData sources: CrossrefPublikationsserver der Universität PotsdamArticle . 2018Data sources: Publikationsserver der Universität Potsdamhttps://dx.doi.org/10.48550/ar...Article . 2018License: arXiv Non-Exclusive DistributionData sources: DataciteÉcole Polytechnique, Université Paris-Saclay: HALArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Eberhard Karls University Tübingen: Publication SystemArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2018Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2018Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1051/0004-6361/201732426&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Conference object , Article , Preprint , Other literature type , Journal 2020Embargo end date: 01 Jan 2020 France, Spain, Spain, SpainPublisher:Sissa Medialab Funded by:ANR | SUPER, UKRI | Materia Oscura: Instrumen..., SNSF | The search for dark matte... +1 projectsANR| SUPER ,UKRI| Materia Oscura: Instrumentation Development to Observe the Invisible ,SNSF| The search for dark matter using CCD detectors (DAMIC) ,NSF| The Search for Light Dark Matter with DAMICA. Aguilar-Arevalo; D. Amidei; D. Baxter; G. Cancelo; B. A. Cervantes Vergara; A. E. Chavarria; J. C. D’Olivo; J. Estrada; F. Favela-Perez; R. Gaïor; Y. Guardincerri; E. W. Hoppe; T. W. Hossbach; B. Kilminster; I. Lawson; S. J. Lee; A. Letessier-Selvon; A. Matalon; P. Mitra; C. T. Overman; A. Piers; P. Privitera; K. Ramanathan; J. Da Rocha; Y. Sarkis; M. Settimo; R. Smida; R. Thomas; J. Tiffenberg; M. Traina; R. Vilar; A. L. Virto;pmid: 33412014
handle: 10261/229942 , 10902/28225
We present constraints on the existence of weakly interacting massive particles (WIMPs) from an 11 kg-day target exposure of the DAMIC experiment at the SNOLAB underground laboratory. The observed energy spectrum and spatial distribution of ionization events with electron-equivalent energies $>$200 eV$_{\rm ee}$ in the DAMIC CCDs are consistent with backgrounds from natural radioactivity. An excess of ionization events is observed above the analysis threshold of 50 eV$_{\rm ee}$. While the origin of this low-energy excess requires further investigation, our data exclude spin-independent WIMP-nucleon scattering cross sections $��_{��-n}$ as low as $3\times 10^{-41}$ cm$^2$ for WIMPs with masses $m_��$ from 7 to 10 GeV$c^{-2}$ . These results are the strongest constraints from a silicon target on the existence of WIMPs with $m_��$$ 6 pages, 4 figures
https://pos.sissa.it... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAArticle . 2020 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAConference object . 2022License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAMémoires en Sciences de l'Information et de la CommunicationConference object . 2021Physical Review LettersArticle . 2020 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useData sources: Crossrefhttps://dx.doi.org/10.48550/ar...Article . 2020License: arXiv Non-Exclusive DistributionData sources: DataciteUniversité de Nantes: HAL-UNIV-NANTESArticle . 2020Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.22323/1.395.0539&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 63 citations 63 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!visibility 42visibility views 42 download downloads 114 Powered bymore_vert https://pos.sissa.it... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAArticle . 2020 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAConference object . 2022License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAMémoires en Sciences de l'Information et de la CommunicationConference object . 2021Physical Review LettersArticle . 2020 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useData sources: Crossrefhttps://dx.doi.org/10.48550/ar...Article . 2020License: arXiv Non-Exclusive DistributionData sources: DataciteUniversité de Nantes: HAL-UNIV-NANTESArticle . 2020Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.22323/1.395.0539&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eu